Results 1 to 10 of about 1,948 (169)
Fading AGNs in Poststarburst Galaxies
The role of active galactic nuclei (AGNs) in quenching galaxies and driving the evolution from star forming to quiescence remains a key question in galaxy evolution.
K. Decker French +6 more
doaj +1 more source
The State of the Molecular Gas in Post-starburst Galaxies
The molecular gas in galaxies traces both the fuel for star formation and the processes that can enhance or suppress star formation. Observations of the molecular gas state can thus point to when and why galaxies stop forming stars.
K. Decker French +9 more
doaj +1 more source
The 2dF Galaxy Redshift Survey: the local E+A galaxy population [PDF]
16 pages, 13 figures, accepted for publication in ...
Blake, Chris +29 more
openaire +5 more sources
Origin of E+A galaxies - I. Physical properties of E+A galaxies formed from galaxy merging and interaction [PDF]
18 pages, 24 figures, accepted by ...
Bekki, K. +3 more
openaire +3 more sources
E+A Galaxies in and Around Nearby Rich Clusters of Galaxies
Abstract We have spectroscopically identified 600 new E+A galaxies and candidates across 16 fields totaling roughly 480 square degrees in the Sloan Digital Sky Survey. E+A galaxies are post-starburst systems that have undergone a significant burst of star formation within the past 1–2 Gyr and are now fully quenched. They comprise a small
Julia Falcone +10 more
openaire +1 more source
DESI Survey Validation Spectra Reveal an Increasing Fraction of Recently Quenched Galaxies at z ∼ 1
We utilize ∼17,000 bright luminous red galaxies (LRGs) from the novel Dark Energy Spectroscopic Instrument Survey Validation spectroscopic sample, leveraging its deep (∼2.5 hr galaxy ^−1 exposure time) spectra to characterize the contribution of recently
David J. Setton +26 more
doaj +1 more source
Activity of Interacting Galaxies Mkn 673: A Close-by “E+A” Galaxy [PDF]
The close-by double nucleus galaxy Mkn 673 shows spectra and colors which are typical for “E+A” cluster galaxies.
W. Kollatschny, K. J. Fricke
openaire +1 more source
Parent Structures in E and SO Galaxies ? [PDF]
Isophote shape and flattening are being used for studying a similarity between elliptical and lenticular galaxies.
R. Michard, F. Simien
openaire +1 more source
Families of galaxies in the e-Re plane [PDF]
Using a complete sample of Virgo cluster galaxies and a larger set of heterogeneous literature data, we show that ellipticals, early-type dwarfs, and bulges of S0s and of spirals form two distinct families in the plane of the effective parameters, R e and μ e . The «ordinary» family is composed of all galaxies fainter than M B ≃−19.3.
CAPACCIOLI M., CAON N., D'ONOFRIO, MAURO
openaire +3 more sources
E+A Galaxies and the Formation of Early‐Type Galaxies atz ∼ 0 [PDF]
30 pages, 11 figures, accepted for publication in ...
Yang, Yujin +4 more
openaire +2 more sources

